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Inflationary cosmology from STM theory of gravity

High Energy Physics - Phenomenology 2010-12-09 v3 General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

I study the power-law and de Sitter expansions for the universe during inflation from the STM theory of gravity. In a de Sitter expansion the additional dimension is related to the cosmological constant. I find from experimental data that the mass of the inflaton field is m2=2/(3Ψ2)m^2=2/(3\Psi^2). In power-law expansion, the fifth coordinate appears to be a dimensionless constant. The interesting here is that the Ψ\Psi-value depends on the initial conditions. I find the 5D line element for this inflationary expansion, which is a function of the classical component of the inflaton.

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Cite

@article{arxiv.hep-ph/0206168,
  title  = {Inflationary cosmology from STM theory of gravity},
  author = {Mauricio Bellini},
  journal= {arXiv preprint arXiv:hep-ph/0206168},
  year   = {2010}
}

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final version